1998/07/31 by Gary A. Williams · 1 citation
Physics and Astronomy · #cond-mat.stat-mech #cond-mat.supr-con #hep-ph
paper · pdf · doi:10.1103/physrevlett.82.1201
published as Phys.Rev.Lett. 82 (1999) 1201-1204 · Version to appear in Phys. Rev. Lett, with a number of corrections and additions
arxiv created 1999/01/18 · arxiv updated 2009/11/30
The distribution of thermally excited vortex loops near a superfluid phase transition is calculated from a renormalized theory. The number density of loops with a given perimeter is found to change from exponential decay with increasing perimeter to algebraic decay as Tc is approached, in agreement with recent simulations of both cosmic strings and high-Tc superconductors. Predictions of the value of the exponent of the algebraic decay at Tc and of critical behavior in the vortex density are confirmed by the simulations, giving strong support to the vortex-folding model proposed by Shenoy.